How the Oblique Drift Instability Alters Solar Wind Heating and Constrains the Distribution of Solar Wind Observations.

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Bibliographic Details
Title: How the Oblique Drift Instability Alters Solar Wind Heating and Constrains the Distribution of Solar Wind Observations.
Authors: Martinović MM; University of Arizona, Lunar and Planetary Laboratory, Tucson, Arizona 85721, USA., Klein KG; University of Arizona, Lunar and Planetary Laboratory, Tucson, Arizona 85721, USA., Ofman L; The Catholic University of America, Washington, DC 20064, USA and Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA., Yogesh; University of Iowa, Department of Physics and Astronomy, Iowa City, Iowa 52242, USA., Howes GG; University of Iowa, Department of Physics and Astronomy, Iowa City, Iowa 52242, USA., Verniero JL; Goddard Space Flight Center, Heliophysics Science Division, NASA, Greenbelt, Maryland 20771, USA., Yoon PH; University of Maryland, Institute for Physical Science and Technology, College Park, Maryland 20742-2431, USA., Verscharen D; University College London, Mullard Space Science Laboratory, Dorking, RH5 6NT, United Kingdom., Alterman BL; Goddard Space Flight Center, Heliophysics Science Division, NASA, Greenbelt, Maryland 20771, USA.
Source: Physical review letters [Phys Rev Lett] 2026 Jun 26; Vol. 136 (25), pp. 255201.
Publication Type: Journal Article
Journal Info: Publisher: American Physical Society Country of Publication: United States NLM ID: 0401141 Publication Model: Print Cited Medium: Internet ISSN: 1079-7114 (Electronic) Linking ISSN: 00319007 NLM ISO Abbreviation: Phys Rev Lett Subsets: MEDLINE; PubMed not MEDLINE
Database: MEDLINE Ultimate
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